Testing gravity of a disformal Kerr black hole in quadratic degenerate higher-order scalar-tensor theories by quasi-periodic oscillations
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Publication:5028763
DOI10.1088/1475-7516/2021/06/043zbMath1485.83070arXiv2103.11788OpenAlexW3138915150MaRDI QIDQ5028763
Jiliang Jing, Zejun Wang, Songbai Chen
Publication date: 10 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2103.11788
Black holes (83C57) Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Quantum field theory on curved space or space-time backgrounds (81T20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Orbital mechanics (70M20) Matrix models and tensor models for quantum field theory (81T32)
Cites Work
- What can we extract from quasiperiodic oscillations?
- Orbital resonances in discs around braneworld Kerr black holes
- Black hole physics. Basic concepts and new developments
- General relativity solutions in modified gravity
- Disforming the Kerr metric
- Testing gravity of a regular and slowly rotating phantom black hole by quasi-periodic oscillations
- On rotating black holes in DHOST theories
- Testing no-hair theorem by quasi-periodic oscillations: the quadrupole of GRO J1655–40
- Hairy black holes in DHOST theories: exploring disformal transformation as a solution generating method
- General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories
- Regular black holes via the Kerr-Schild construction in DHOST theories
- Hairy rotating black holes in cubic Galileon theory